Jacobi coordinates

File:Two-body Jacobi coordinates.JPG; Jacobi coordinates are \boldsymbol{R}=\frac {m_1}{M} \boldsymbol{x}_1 + \frac {m_2}{M} \boldsymbol{x}_2 and \boldsymbol{r} = \boldsymbol{x}_1 - \boldsymbol{x}_2 with M = m_1+m_2 .{{cite book |title=Differential Equations |author=David Betounes |url=https://archive.org/details/differentialequa0000beto |url-access=registration |isbn=0-387-95140-7 |page=58; Figure 2.15 |date=2001 |publisher=Springer}}]]

File:Jacobi coordinates — illustration for four bodies.svg

In the theory of many-particle systems, Jacobi coordinates often are used to simplify the mathematical formulation. These coordinates are particularly common in treating polyatomic molecules and chemical reactions,

{{cite book |title=Theory and application of quantum molecular dynamics |author= John Z. H. Zhang |url=https://books.google.com/books?id=b8AzpUPopqQC&pg=PA104 |page=104 |isbn=981-02-3388-4 |date=1999 |publisher=World Scientific}}

and in celestial mechanics.

For example, see {{cite book |title=Capture Dynamics and Chaotic Motions in Celestial Mechanics |author= Edward Belbruno |url=https://books.google.com/books?id=dK-fl0KrOEIC&pg=PA9 |page=9 |isbn=0-691-09480-2 |date=2004 |publisher=Princeton University Press}}

An algorithm for generating the Jacobi coordinates for N bodies may be based upon binary trees.

{{cite book |title=Classical and celestial mechanics |author= Hildeberto Cabral, Florin Diacu |chapter-url=https://books.google.com/books?id=q1emz4C4lYQC&pg=PA230 |page=230 |chapter=Appendix A: Canonical transformations to Jacobi coordinates |isbn=0-691-05022-8 |publisher=Princeton University Press |date=2002}}

In words, the algorithm may be described as follows:

We choose two of the N bodies with position coordinates xj and xk and we replace them with one virtual body at their centre of mass. We define the relative position coordinate rjk = xj − xk.

We then repeat the process with the N − 1 bodies consisting of the other N − 2 plus the new virtual body. After N − 1 such steps we will have Jacobi coordinates consisting of the relative positions and one coordinate giving the position of the last defined centre of mass.

For the N-body problem the result is:{{cite book |title=Advanced electromagnetism and vacuum physics |author=Patrick Cornille |page=102 |chapter-url=https://books.google.com/books?id=y8sSFTDkQ20C&pg=PA102 |chapter=Partition of forces using Jacobi coordinates |isbn=981-238-367-0 |date=2003 |publisher=World Scientific}}

:\boldsymbol{r}_j= \frac{1}{m_{0j}} \sum_{k=1}^j m_k\boldsymbol {x}_k \ - \ \boldsymbol{x}_{j+1}\ , \quad j \in \{1, 2, \dots, N-1\}

:\boldsymbol{r}_N= \frac{1}{m_{0N}} \sum_{k=1}^N m_k\boldsymbol {x}_k \ ,

with

:m_{0j} = \sum_{k=1}^j \ m_k \ .

The vector \boldsymbol{r}_N is the center of mass of all the bodies and \boldsymbol{r}_1 is the relative coordinate between the particles 1 and 2:

The result one is left with is thus a system of N-1 translationally invariant coordinates \boldsymbol{r}_1, \dots, \boldsymbol{r}_{N-1} and a center of mass coordinate \boldsymbol{r}_N, from iteratively reducing two-body systems within the many-body system.

This change of coordinates has associated Jacobian equal to 1.

If one is interested in evaluating a free energy operator in these coordinates, one obtains

:H_0=-\sum_{j=1}^N\frac{\hbar^2}{2 m_j}\, \nabla^2_{\boldsymbol{x}_j} = -\frac{\hbar^2}{2 m_{0N}}\,\nabla^2_{\boldsymbol{r}_{N}}\!-\frac{\hbar^2}{2}\sum_{j=1}^{N-1}\!\left(\frac{1}{m_{j+1}}+\frac{1}{m_{0j}}\right)\nabla^2_{\boldsymbol{r}_j}

In the calculations can be useful the following identity

:\sum_{k=j+1}^N \frac{m_k}{m_{0k}m_{0k-1}}=\frac{1}{m_{0j}}-\frac{1}{m_{0N}}.

References